Rm. Williams et al., Supernova remnants in the magellanic clouds. III. An X-ray atlas of large magellanic cloud supernova remnants, ASTROPH J S, 123(2), 1999, pp. 467-485
We have used archival ROSAT data to present X-ray images of 31 supernova re
mnants (SNRs) in the Large Magellanic Cloud (LMC). We have classified these
remnants according to their X-ray morphologies, into the categories of she
ll-type, diffuse face, centrally brightened, point-source-dominated, and ir
regular. We suggest possible causes of the X-ray emission for each category
and for individual features of some of the SNRs.